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M

M. Cano Díaz

Researcher at National Autonomous University of Mexico

Publications -  4
Citations -  1348

M. Cano Díaz is an academic researcher from National Autonomous University of Mexico. The author has contributed to research in topics: Spectral resolution & Population. The author has an hindex of 4, co-authored 4 publications receiving 1203 citations.

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The Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory

Franco D. Albareti, +336 more
- 05 Aug 2016 - 
TL;DR: Data Release 13 (DR13) as mentioned in this paper is the first data release from SDSS-IV, which contains new data, reanalysis of existing data sets and, like all SDSs data releases, is inclusive of previously released data.
Journal ArticleDOI

The 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory

Franco D. Albareti, +400 more
- 08 Dec 2017 - 
TL;DR: Data Release 13 (DR13) as discussed by the authors provides the first 1390 spatially resolved integral field unit observations of nearby galaxies from the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2), Mapping Nearby Galaxies at APO (MaNGA), and the Extended Baryon Oscillation Spectroscopic Survey (eBOSS).
Journal ArticleDOI

CALIFA, the Calar Alto Legacy Integral Field Area survey - III. Second public data release

Sebastián F. Sánchez, +65 more
- 01 Jan 2013 - 
TL;DR: The second public data release (DR2) of the Calar Alto Legacy Integral Field Area (CALIFA) survey as discussed by the authors contains over 1.5 million spectra.
Journal ArticleDOI

CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third Public data release

Sebastián F. Sánchez, +62 more
- 08 Apr 2016 - 
TL;DR: The third public data release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey as mentioned in this paper contains 1576 datacubes, including ~1.5 million independent spectra.